Chiral Anomaly in Contorted Spacetimes
arXiv:gr-qc/9704051 · doi:10.1023/A:1026653314045
Abstract
The Dirac equation in Riemann-Cartan spacetimes with torsion is reconsidered. As is well-known, only the axial covector torsion , a one-form, couples to massive Dirac fields. Using diagrammatic techniques, we show that besides the familiar Riemannian term only the Pontrjagin type four-form does arise additionally in the chiral anomaly, but not the Nieh-Yan term , as has been claimed recently. Implications for cosmic strings in Einstein-Cartan theory as well as for Ashtekar's canonical approach to quantum gravity are discussed.
17 pages, REVTEX
References in corpus (1)
Cited by in corpus (10)
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